SOHO EIT Analysis Proposal Submission Form

Mailing address:

E-mail address:

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Topic:
Abundances Acoustic Waves Active Regions Alfven Waves Arcades Arches Background Corona BOUDINE Bright Points Brightness Distribution Brightness Temperature Calcium Calibration Campaigns CCD CDS CELIAS Chemical Composition Chromosphere Chromospheric Network CME Coronagraph Coronal Condensations Coronal Heating Coronal Holes Coronal Loops Coronal Mass Ejection Coronal Plasma Cosmic Rays COSTEP Current Sheets Data Compression Data Processing Density Density Distribution Dissipative Processes EIT Electron Beams Electron Density Electron Distribution Electron Temperature Emission Lines Energy Balance Energy Transfer ERNE EUV EUV Flux EUV Indices EUV Lines EUV Proxies EUV Sources EUV Spectrum F-Corona Fe IX-X 17.1 nm Fe XII 19.5 nm Fe XV 28.4 nm Filaments Flares Flat Field Forbidden Lines Gamma-Ray Bursts GOLF Grid Grid Removal Ground-Based Coordination Ground-Based Observatories He II 30.4 nm Heat Flow Heliosphere Helium High Resolution Imaging Hydrogen Image Image Processing Imaging In Situ Measurements Interplanetary Dust Interplanetary Magnetic Field Interplanetary Space IR Lines IR Spectrum Iron K-Corona Large-Scale Structure LASCO Line Intensities Line Profiles Magnesium Magnetic Fields Magnetic Flux Tubes Magnetic Reconnection Magnetohydrodynamics Magnetosphere Mass Ejection MDI MHD Waves Microwave Bursts Microwave Radiation Models Morphology Multilayers Nanoflares Onboard Software Oscillations Particles Photosphere Plasma Plasma Diagnostics Plasma Waves Pointing Polar Holes Polar Plumes Polar Regions Polarimetry Polarization Prominences Predictions Quiet Sun Radiative Transfer Radio Bursts Radio Spectrum Radioheliography Remote Sensing Resonance Lines Rocket Rotation Scattering Shock Waves Soft X-Rays Software SOHO SOI Solar Activity Solar Cycle Solar Dynamo Solar Eclipses Solar Indices Solar Spectrum Solar-Terrestrial Relations Solar Wind Spectral Lines Spectrography Spectrometers Spicules Spikes Statistics Streamers SUMER Sunspots SWAN SXT Synoptic Maps Telemetry Temperature Temperature Diagnostic Temperature Distribution Transients Transition Region Turbulence ULYSSES UV Lines UV Spectrum UVCS Velocities VIRGO Waves X-rays Flares X-Rays YOHKOH

If none of these topics are appropriate, please enter your own:

Proposal Title

Please describe what you propose to do, with which EIT data, and with what correlative data (if any). This proposal need be only a few paragraphs in length.

Finally, please include the names of any EIT team members with whom you propose to work (optional, but until 1997 September, all proposals will be expected to involve a collaboration with an EIT Consortium member). If you are already in the EIT Consortium, please check the EIT Consortium button.

I am an EIT Consortium member: Yes. No.

You must click the "submit" button in order to enter your proposal. Thank you.